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University Physics I - Classical Mechanics, 2019

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8.7. ADVANCED TOPICS 179<br />

8.7 Advanced Topics<br />

8.7.1 Staying on track<br />

(This example studies a situation that you could easily setup experimentally at home (you can use<br />

a whole sphere instead of a half-sphere!), although to get the numbers to work out you really need<br />

to make sure that the friction between the surface and the object you choose is truly negligible.<br />

Essentially the same mathematical approach could be used to study the problem of a skier going<br />

over a mogul, or a car losing contact with the road if it is going too fast over a hill.)<br />

A small object is placed at the top of a smooth (frictionless) dome shaped like a half-sphere of<br />

radius R, and given a small push so it starts sliding down the dome, initially moving very slowly<br />

(v i ≃ 0), but picking up speed as it goes, until at some point it flies off the surface.<br />

(a) At that point, when the object loses contact with the surface, what is the angle that its position<br />

vector (with origin at the center of the sphere) makes with the vertical?<br />

(b) How far away from the sphere does the object land?<br />

F n<br />

sb<br />

θ<br />

θ max<br />

θ<br />

θ<br />

F G<br />

Eb<br />

(a)<br />

(b)<br />

Figure 8.8: An object (small block) sliding on a hemispherical dome. The drawing (a) shows the angle<br />

θ max at which the object flies off (red dashed line), and a smaller, generic angle θ. The drawing (b) shows<br />

the free-body diagram corresponding to the angle θ.<br />

Solution<br />

(a) As we saw in Section 8.4, in order to get an object to move along an arc of a circle, a centripetal<br />

force of magnitude mv 2 /r is required. As long as our object is in contact with the surface, the<br />

forces acting on it are the normal force (which points along the radial direction, so it makes a<br />

negative contribution to the centrifugal force) and gravity, which has a component mg cos θ along<br />

the radius, towards the center of the circle (see Figure 8.8(b), the dashed light blue line). So, the<br />

centripetal force equation reads<br />

mv 2<br />

R = mg cos θ − F n (8.46)

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